The galaxy appears to be an elongated, cigar-shaped structure. Its light profile suggests a relatively smooth distribution with a dominant central bulge. There may be a hint of a faint disk structure, but it does not appear well-defined. The galaxy's color gradient shows bluer hues towards the outer regions and redder tones in the central bulge, which could indicate active star formation in the outer areas and an older stellar population in the core. There is no visually apparent evidence of a major merger event or significant tidal disturbances, but a minor disturbance or potential interaction cannot be entirely ruled out given the low image resolution. Overall, the galaxy is likely a spiral transitioning to lenticular, or perhaps an elliptical galaxy exhibiting characteristics of past star formation.
