The galaxy appears as a relatively smooth, single object. It exhibits a shape that falls between perfectly round and elongated, with no obvious spiral arm structures visible. A slight elongation towards what would be considered a cigar shape is present. The color profile shows a general redder hue, indicating a population of older stars and suggesting lower levels of ongoing star formation. There are no strong indicators of any major merging events or significant tidal disturbances affecting the overall galactic structure. A mild level of disturbance may be indicated, but it is not distinctly visible.
