This galaxy presents as a lenticular or elliptical type, characterized by a smooth, relatively featureless light distribution. The core exhibits a concentrated, yellowish hue suggesting an older stellar population and a lack of significant recent star formation. The galaxy is elongated, with the major axis clearly exceeding the minor axis, indicating a degree of flattening. There appears to be a subtle disk component, though it lacks distinct spiral arms. Some possible minor disturbances are present in the disk. The outer regions display a gradient of decreasing surface brightness. There are faint hints of bluer light in the outer regions of the galaxy possibly pointing to a small amount of ongoing star formation. The galaxy is relatively isolated, showing no immediate signs of major mergers or interactions with other large galaxies.
