The galaxy presents as a disk-shaped structure, viewed at a high inclination relative to our line of sight. The central region exhibits a noticeable bulge, appearing more luminous and concentrated than the outer regions. The overall color profile suggests a dominant population of older stars within the central bulge, exhibiting a yellowish hue, possibly indicative of diminished star formation in this area. Fainter, bluer regions are visible at the extreme edges of the disk, indicating the potential presence of younger, hotter stars associated with ongoing or recent star formation, although such activity appears to be at a relatively low rate. The galaxy appears relatively isolated, without any obvious signs of major gravitational disturbance or interactions. Faint spiral arm structures may be present but are not clearly defined. The galaxy's major axis appears significantly elongated relative to its minor axis, consistent with a classification as a late-type spiral or lenticular galaxy seen edge-on.
