The galaxy appears as an elongated, cigar-shaped structure. It has a relatively smooth morphology, with a dominant bulge that is not very large compared to the galaxy. There is a subtle disk with hints of faint spiral arm structure, though they are not well-defined. The color of the galaxy is notably redder in the bulge region, transitioning to bluer hues in the outer disk. The redder color of the bulge suggests an older stellar population, while the bluer disk indicates ongoing or recent star formation. There do not appear to be any major distortions or signs of recent merging activity, although there may be a minor disturbance due to asymmetry or subtle irregularities in the outer regions. The overall light profile suggests a relatively low mass system. The galaxy shows very little visible dust absorption.
