The galaxy presents as an elongated, disk-like structure, viewed at a near edge-on inclination. A central bulge region is faintly discernible, appearing more diffuse than a distinct core. The overall color gradient suggests a population of older stars dominates the bulge, emitting light that skews towards the redder end of the spectrum. The disk component exhibits a bluer hue, indicative of ongoing or recent star formation. While no distinct spiral arm structure is readily apparent, the slight irregularities and patchy distribution of bluer regions within the disk imply the presence of star-forming regions. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Its shape approximates an elongated, somewhat cigar-like form, lacking pronounced features. The lack of more distinct features and somewhat muted colors suggest that star formation is slow.