The galaxy presents a somewhat elongated, cigar-shaped morphology. Its central region exhibits a bright, yellowish-white core, likely indicative of an older stellar population. Moving outward from the core, the light gradually diminishes. There is a suggestion of a flattened structure, though any spiral arm details are not obviously visible.

The overall appearance suggests a relatively smooth distribution of light. The galaxy displays a reddish hue, consistent with a galaxy where star formation rates are low. This is further supported by the galaxy’s apparent lack of prominent blue regions, which typically indicate the presence of young, hot stars associated with recent or ongoing star formation. The light distribution exhibits no significant distortions or irregularities, implying a generally relaxed dynamical state. There appears to be a small companion galaxy at close proximity to the galaxy being observed.
